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Longer titles found: Habitability of binary star systems (view), Binary Star (hip-hop group) (view)

searching for binary star 99 found (2160 total)

Made in Abyss (3,954 words) [view diff] case mismatch in snippet view article find links to article

digital outlets. An action role-playing game, titled Made in Abyss: Binary Star Falling into Darkness (メイドインアビス闇を目指した連星, Meido in Abisu Yami o Mezashita

WZ Andromedae (520 words) [view diff] exact match in snippet view article find links to article

WZ Andromedae (abbreviated to WZ And) is an eclipsing binary star in the constellation Andromeda. Its maximum apparent visual magnitude is 11.6, but drops

KPD 1930+2752 (531 words) [view diff] exact match in snippet view article find links to article

KPD 1930+2752 is a binary star system including a subdwarf B star and a probable white dwarf with relatively high mass. Due to the nature of this astronomical

Position angle (377 words) [view diff] exact match in snippet view article find links to article

pole. As the example illustrates, if one were observing a hypothetical binary star with a PA of 30°, that means an imaginary line in the eyepiece drawn

DS Andromedae (744 words) [view diff] exact match in snippet view article find links to article

DS Andromedae (often abbreviated to DS And) is an eclipsing binary star in the constellation Andromeda and a member of the open cluster NGC 752. Its maximum

Psi6 Aurigae (511 words) [view diff] exact match in snippet view article find links to article

Psi6 Aurigae is a spectroscopic binary star system in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from ψ6

Kepler-453b (169 words) [view diff] no match in snippet view article find links to article

Kepler-453b is a transiting circumbinary exoplanet in the binary-star system Kepler-453. It orbits the binary system in the habitable zone every 240.5

QR Andromedae (721 words) [view diff] exact match in snippet view article find links to article

QR Andromedae (often abbreviated to QR And) is an eclipsing binary star in the constellation Andromeda. Its maximum apparent visual magnitude is 12.16

NGC 2899 (565 words) [view diff] exact match in snippet view article find links to article

significant equatorial structure. This shape is believed to result from a binary star system. The mean expansion rate is 43 to 56 km/s, with high velocity

KX Andromedae (589 words) [view diff] exact match in snippet view article find links to article

KX Andromedae (often abbreviated to KX And) is a spectroscopic binary star in the constellation Andromeda. Its apparent visual magnitude varies between

R Canis Majoris (717 words) [view diff] exact match in snippet view article find links to article

R Canis Majoris is an eclipsing interacting binary star system in the constellation Canis Major. It varies from magnitude 5.7 to 6.34. The system is unusual

CN Andromedae (607 words) [view diff] exact match in snippet view article find links to article

CN Andromedae (CN And) is an eclipsing binary star in the constellation Andromeda. Its maximum apparent visual magnitude is 9.62 and drops down to a minimum

AC Herculis (722 words) [view diff] exact match in snippet view article find links to article

AC Herculis, is an RV Tauri variable and spectroscopic binary star in the constellation of Hercules. It varies in brightness between apparent magnitudes

HD 59686 Ab (226 words) [view diff] exact match in snippet view article find links to article

Ab is an exoplanet that orbits the giant star HD 59686 A in a close binary star system. It has a nearly circular orbit with a period of 300 days and

List of nearest known black holes (1,311 words) [view diff] exact match in snippet view article find links to article

solution has a mass of 5.6 MSol. 4,700±800 1.44±0.25 A0620-00 (V616 Mon) Binary star system with orbit t=7.75 h 06h 22m 44.503s −00° 20′ 44.72″ 1986 A BH

F Centauri (419 words) [view diff] exact match in snippet view article find links to article

F Centauri is a suspected astrometric binary star system in the southern constellation of Centaurus. It has a reddish hue and is visible to the naked

HD 174569 (431 words) [view diff] exact match in snippet view article find links to article

HD 174569 is a spectroscopic binary star system in the equatorial constellation of Aquila. Based on stellar parallax measurements by Gaia, it is about

BX Andromedae (715 words) [view diff] exact match in snippet view article find links to article

BX Andromedae (BX And) is an eclipsing binary star in the constellation Andromeda. Its maximum apparent visual magnitude is 8.87. Within a cycle of approximately

KIC 9832227 (781 words) [view diff] exact match in snippet view article find links to article

KIC 9832227 is a contact binary star system in the constellation Cygnus, located about 2,060 light-years away. It is also identified as an eclipsing binary

BB Doradus (318 words) [view diff] exact match in snippet view article find links to article

BB Dor is a cataclysmic variable, a pre-nova star, thus a close pair binary star system. It is composed of a red dwarf and a white dwarf. Observations

NGC 6881 (135 words) [view diff] exact match in snippet view article find links to article

light-year from one tip to the other. The symmetry could be due to a binary star at the nebula's centre. "NGC 6881". SIMBAD. Centre de données astronomiques

KOI-74 (507 words) [view diff] exact match in snippet view article find links to article

KOI-74 (KIC 6889235) is an eclipsing binary star in the constellation of Cygnus. The primary star is an A-type main-sequence star with a temperature of

4 Sagittarii (454 words) [view diff] exact match in snippet view article find links to article

4 Sagittarii is a suspected astrometric binary star system in the zodiac constellation of Sagittarius, located approximately 390 light years away based

HD 10307 (868 words) [view diff] exact match in snippet view article find links to article

HD 10307 (HR 483) is a spectroscopic binary star in the constellation Andromeda. The primary is similar to the Sun in mass, temperature and metal content

AB Doradus (1,013 words) [view diff] exact match in snippet view article find links to article

four components consisting of a pair of binary star systems separated by an angle of about 9″. The binary star AB Doradus Ba/Bb orbits the primary AB Doradus

Kepler-451 (584 words) [view diff] exact match in snippet view article find links to article

and abbreviated to 2M1938+4603) is an eclipsing post-common envelope binary star system that comprises two stars, a pulsating subdwarf B star and a small

35 Cygni (647 words) [view diff] exact match in snippet view article find links to article

35 Cygni is a spectroscopic binary star in the constellation Cygnus. Its apparent magnitude is 5.18. Located around 1,000 parsecs (3,300 ly) distant,

4U 0614+091 (121 words) [view diff] exact match in snippet view article find links to article

4U 0614+091 is a low-mass X-ray binary star system which features a neutron star and a low-mass companion star. The binary system lies 10,000 light-years

6 Andromedae (720 words) [view diff] exact match in snippet view article find links to article

6 Andromedae is an astrometric binary star system in the northern constellation of Andromeda. The designation comes from the star catalogue of John Flamsteed

C3 Centauri (523 words) [view diff] exact match in snippet view article find links to article

C3 Centauri is a suspected astrometric binary star system in the southern constellation of Centaurus. It has an orange hue and is dimly visible to the

35 Cygni (647 words) [view diff] exact match in snippet view article find links to article

35 Cygni is a spectroscopic binary star in the constellation Cygnus. Its apparent magnitude is 5.18. Located around 1,000 parsecs (3,300 ly) distant,

Gliese 15 Ac (415 words) [view diff] exact match in snippet view article find links to article

star Gliese 15 A (Groombridge 34 A, GX Andromedae), which is part of a binary star system located about 11.6 light-years from the Sun. The planet was first

10 Andromedae (433 words) [view diff] exact match in snippet view article find links to article

10 Andromedae, abbreviated 10 And, is an astrometric binary star system in the northern constellation of Andromeda. 10 Andromedae is the Flamsteed designation

IC 348 (416 words) [view diff] exact match in snippet view article find links to article

angular diameter of 20″. The most massive stars in the cluster are the binary star system BD+31°643, which has a combined spectral class of B5. Based upon

V446 Herculis (457 words) [view diff] exact match in snippet view article find links to article

arise from the star itself. Like all novae, V446 Herculis is a close binary star system with a "donor" star transferring matter to its white dwarf companion

K Centauri (430 words) [view diff] exact match in snippet view article find links to article

K Centauri is a possible binary star in the southern constellation of Centaurus. It has a white hue and is bright enough to be visible to the naked eye

HD 23089 (341 words) [view diff] exact match in snippet view article find links to article

HD 23089 is a spectroscopic binary star in the northern constellation of Camelopardalis. Based on stellar parallax measurements made by Hipparcos, the

HD 76728 (475 words) [view diff] exact match in snippet view article find links to article

HD 76728 is a suspected astrometric binary star system in the constellation Carina. It has the Bayer designation c Carinae; HD 76728 is the identifier

Xi Cancri (768 words) [view diff] exact match in snippet view article find links to article

Xi Cancri (ξ Cancri, abbreviated Xi Cnc, ξ Cnc) is a spectroscopic binary star system in the zodiac constellation of Cancer. It is visible to the naked

V446 Herculis (457 words) [view diff] exact match in snippet view article find links to article

arise from the star itself. Like all novae, V446 Herculis is a close binary star system with a "donor" star transferring matter to its white dwarf companion

Kepler-560b (237 words) [view diff] exact match in snippet view article find links to article

Kepler-560 Bb, is a confirmed exoplanet orbiting the secondary star of the binary star system Kepler-560. It is only 287 light-years away. Though not listed

V3903 Sagittarii (726 words) [view diff] exact match in snippet view article find links to article

known as 11 Sagittarii, or its abbreviation 11 Sgr) is an eclipsing binary star system in the constellation Sagittiarus. It creates an H II region LBN

HD 34790 (448 words) [view diff] exact match in snippet view article find links to article

HD 34790 is a double-lined spectroscopic binary star system in the northern constellation of Auriga. It has a combined apparent magnitude of 5.66, which

Kepler-89 (523 words) [view diff] exact match in snippet view article find links to article

is a star with four confirmed planets. Kepler-89 is a possible wide binary star. The discovery of four planets orbiting the star was announced October

R145 (1,082 words) [view diff] exact match in snippet view article find links to article

R145 (HD 269928) is a spectroscopic binary star in the Tarantula Nebula in the Large Magellanic Cloud located in the constellation Dorado. Both components

HD 102776 (786 words) [view diff] exact match in snippet view article find links to article

known by its Bayer designation j Centauri, is a suspected astrometric binary star system in the southern constellation of Centaurus. It has a blue-white

Messier 73 (823 words) [view diff] exact match in snippet view article find links to article

2170±22, and 2290±24 light-years from the Sun, with the second being a binary star. M73 was discovered by Charles Messier in 1780 who originally described

OGLE-TR-113 (431 words) [view diff] exact match in snippet view article find links to article

OGLE-TR-113 is a dim, distant magnitude 16 binary star in the star fields of the constellation Carina. Because of its distance of about 1170 light years

HD 34790 (448 words) [view diff] exact match in snippet view article find links to article

HD 34790 is a double-lined spectroscopic binary star system in the northern constellation of Auriga. It has a combined apparent magnitude of 5.66, which

R145 (1,082 words) [view diff] exact match in snippet view article find links to article

R145 (HD 269928) is a spectroscopic binary star in the Tarantula Nebula in the Large Magellanic Cloud located in the constellation Dorado. Both components

OGLE-TR-113 (431 words) [view diff] exact match in snippet view article find links to article

OGLE-TR-113 is a dim, distant magnitude 16 binary star in the star fields of the constellation Carina. Because of its distance of about 1170 light years

12 Persei (482 words) [view diff] exact match in snippet view article find links to article

12 Persei (12 Per) is a double-lined spectroscopic binary star system in the northern constellation Perseus. Its combined apparent magnitude is 4.94,

HD 112028 (426 words) [view diff] exact match in snippet view article find links to article

main sequence stars. HD 112028 and HD 112014 together are known as the binary star Struve 1694. Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia

HD 38282 (701 words) [view diff] exact match in snippet view article find links to article

HD 38282 (R144, BAT99-118, Brey 89) is a massive spectroscopic binary star in the Tarantula Nebula (Large Magellanic Cloud), consisting of two hydrogen-rich

Winnecke 4 (811 words) [view diff] exact match in snippet view article find links to article

parsecs (470 ± 1 light-year) respectively. HD 238108 is itself a genuine binary star, with an 18th magnitude white dwarf companion 5 arcseconds away and a

36 G. Doradus (637 words) [view diff] exact match in snippet view article find links to article

36 G. Doradus (HD 40409) is a suspected astrometric binary star system in the southern constellation of Dorado. It is a faint system but visible to the

Kepler-411 (1,048 words) [view diff] exact match in snippet view article find links to article

Kepler-411 is a binary star system. Its primary star Kepler-411A is a K-type main-sequence star, orbited by the red dwarf star Kepler-411B on a wide orbit

Xi Cygni (549 words) [view diff] exact match in snippet view article find links to article

ξ Cygni (Latinised as Xi Cygni) is a spectroscopic binary star in the constellation Cygnus, made up of a K-type supergiant star (primary) and an A-type

Winnecke 4 (811 words) [view diff] exact match in snippet view article find links to article

parsecs (470 ± 1 light-year) respectively. HD 238108 is itself a genuine binary star, with an 18th magnitude white dwarf companion 5 arcseconds away and a

Eridanus (constellation) (1,498 words) [view diff] exact match in snippet view article

name, which means "the footstool". Theta Eridani, called Acamar, is a binary star with blue-white components, distinguishable in small amateur telescopes

HD 22663 (372 words) [view diff] exact match in snippet view article find links to article

HD 22663 (y Eridani) is a candidate astrometric binary star system in the equatorial constellation of Eridanus. It is visible to the naked eye with an

AG Virginis (1,035 words) [view diff] exact match in snippet view article find links to article

AG Virginis is an eclipsing binary star system in the equatorial constellation of Virgo. With a maximum apparent visual magnitude of 8.51 it is too faint

HD 91190 (374 words) [view diff] exact match in snippet view article find links to article

HD 91190 is a suspected astrometric binary star system in the northern circumpolar constellation of Draco. It is faintly visible to the naked eye, having

HD 110073 (516 words) [view diff] exact match in snippet view article find links to article

a radial velocity of +15 km/s. This is a single-lined spectroscopic binary star system that belongs to the Pleiades stream. As of 2011, the pair had

KOI-81 (550 words) [view diff] exact match in snippet view article find links to article

KOI-81 is an eclipsing binary star in the constellation of Cygnus. The primary star is a late B-type or early A-type main-sequence star with a temperature

HD 326823 (772 words) [view diff] exact match in snippet view article find links to article

HD 326823, also known as V1104 Scorpii, is a binary star containing a unique emission-line star, which is in the midst of transitioning to a nitrogen-rich

HD 326823 (772 words) [view diff] exact match in snippet view article find links to article

HD 326823, also known as V1104 Scorpii, is a binary star containing a unique emission-line star, which is in the midst of transitioning to a nitrogen-rich

NGC 2360 (531 words) [view diff] exact match in snippet view article find links to article

Gamma Canis Majoris and less than one degree northwest of the eclipsing binary star R Canis Majoris; it has a combined apparent magnitude of 7.2. It is 13

WZ Cephei (322 words) [view diff] exact match in snippet view article find links to article

WZ Cephei is an eclipsing binary star of W Ursae Majoris-type in the constellation of Cepheus, located 880 light years away from the Sun. The stars orbit

12 Aquarii (339 words) [view diff] exact match in snippet view article find links to article

velocity of +1.1 km/s. The magnitude 5.88 primary, component A, is itself a binary star with a separation of 0.05″–0.07″ and an orbital period of around 18.5 yr

U Coronae Borealis (201 words) [view diff] exact match in snippet view article find links to article

U Coronae Borealis (U CrB) is an Algol-type eclipsing binary star system in the constellation Corona Borealis. Its apparent magnitude varies between 7

GCIRS 16SW (696 words) [view diff] exact match in snippet view article find links to article

GCIRS 16SW, also known as S97, is a contact binary star located in the Galactic Center. It is composed of two hot massive stars of equal size that orbit

WR 22 (1,401 words) [view diff] exact match in snippet view article find links to article

WR 22, also known as V429 Carinae or HR 4188, is an eclipsing binary star system in the constellation Carina. The system contains a Wolf-Rayet (WR) star

LH 54-425 (863 words) [view diff] exact match in snippet view article find links to article

LH 54-425 is a spectroscopic binary star system in the LH 54 OB association within the Large Magellanic Cloud in the constellation Dorado. The OB association

U Coronae Borealis (201 words) [view diff] exact match in snippet view article find links to article

U Coronae Borealis (U CrB) is an Algol-type eclipsing binary star system in the constellation Corona Borealis. Its apparent magnitude varies between 7

NGC 6025 (669 words) [view diff] exact match in snippet view article find links to article

compared to the Sun; more so than the Hyades cluster. Seven spectroscopic binary star systems have been identified. Only one blue straggler has been found

FL Lyrae (623 words) [view diff] exact match in snippet view article find links to article

FL Lyrae is the variable star designation for an eclipsing binary star system in the northern constellation of Lyra. The combined apparent magnitude of

Lambda Hydrae (717 words) [view diff] exact match in snippet view article find links to article

λ Hydrae, Latinised as Lambda Hydrae, is a spectroscopic binary star in the constellation Hydra. Its apparent magnitude is 3.61 Located around 33.3 parsecs

GRS 1915+105 (804 words) [view diff] exact match in snippet view article find links to article

GRS 1915+105 or V1487 Aquilae is an X-ray binary star system containing a main sequence star and a black hole. Transfer of material from the star to the

6 Draconis (580 words) [view diff] exact match in snippet view article find links to article

6 Draconis is a single-lined spectroscopic binary star system in the northern constellation of Draco, located about 430 light years away from the Sun

Delta Cassiopeiae (1,142 words) [view diff] exact match in snippet view article find links to article

Cassiopeiae (δ Cassiopeiae, abbreviated Delta Cas, δ Cas) is an eclipsing binary star system in the northern circumpolar constellation of Cassiopeia. Based

HD 126053 (842 words) [view diff] exact match in snippet view article find links to article

It shares a common proper motion through space with the spectroscopic binary star system HD 122742, and in the past the three may have formed a triple

HD 42818 (688 words) [view diff] exact match in snippet view article find links to article

HD 42818 is a suspected astrometric binary star system in the northern circumpolar constellation of Camelopardalis. It is visible to the naked eye with

Wild Duck Cluster (718 words) [view diff] exact match in snippet view article find links to article

plus 29 lower probability members. The former include two eclipsing binary star systems. The cluster is located 6.8 kpc (22,000 ly) from the Galactic

Eta Andromedae (787 words) [view diff] exact match in snippet view article find links to article

Eta Andromedae, also named Kui, is a spectroscopic binary star system in the northern constellation of Andromeda. It consists of two G-type evolved stars

111 Herculis (605 words) [view diff] exact match in snippet view article find links to article

111 Herculis is a suspected astrometric binary star system located 92 light years from the Sun in the northern constellation Hercules. It is visible to

Senim Silla (174 words) [view diff] case mismatch in snippet view article find links to article

from Pontiac, Michigan, best known as one of the two MCs in rap duo Binary Star, along with One Be Lo. Senim Silla co-hosted the Foreally Show with lifelong

7 Tauri (546 words) [view diff] exact match in snippet view article find links to article

equivalent to a distance of around 593 light years from the Sun. 7 Tauri is a binary star with two nearly equal components about 0.7″ apart, designated as A and

14 Aquilae (524 words) [view diff] exact match in snippet view article find links to article

14 Aquilae is a probable spectroscopic binary star system in the equatorial constellation of Aquila. 14 Aquilae is the Flamsteed designation though it

20 Cancri (381 words) [view diff] exact match in snippet view article find links to article

20 Cancri is an astrometric binary star system in the constellation Cancer, located about 372 light-years away from the Sun. This system has the Bayer

51 Andromedae (784 words) [view diff] exact match in snippet view article find links to article

of the mythological, chained-to-the-rocks princess, the other being binary star system Gamma Andromedae. At an estimated age of 1.7 billion years, this

U Lacertae (828 words) [view diff] exact match in snippet view article find links to article

U Lacertae is a spectroscopic binary star in the constellation Lacerta. Despite being in the constellation of Lacerta, U Lacertae is considered to be

GG Lupi (514 words) [view diff] exact match in snippet view article find links to article

GG Lupi is an eclipsing binary star in the southern constellation of Lupus. Most of the time it is a magnitude 5.6 object, making it faintly visible to

WASP-11b/HAT-P-10b (686 words) [view diff] exact match in snippet view article find links to article

dividing line between the class I and class II planets. The planet is in a binary star system, the second star is WASP-11 B, with a mass 0.34 ± 0.05 of the

15 Orionis (600 words) [view diff] exact match in snippet view article find links to article

15 Orionis is a suspected astrometric binary star system in the equatorial constellation of Orion, near the border with Taurus. It is visible to the naked

Theta Carinae (903 words) [view diff] exact match in snippet view article find links to article

θ Carinae, Latinized as Theta Carinae, is a spectroscopic binary star in the southern constellation of Carina. With an apparent visual magnitude of 2

NGC 6633 (309 words) [view diff] exact match in snippet view article find links to article

chemically peculiar star - NGC 6633 48 (BD+06 3755). The 8th-magnitude binary star HD 169959 (NGC 6633 58) is within the line-of-sight of the open cluster

UW Coronae Borealis (355 words) [view diff] exact match in snippet view article find links to article

Coronae Borealis, also known as MS 1603.6+2600, is a low-mass X-ray binary star system in the constellation Corona Borealis. Astronomer Simon Morris

Delta Trianguli (840 words) [view diff] exact match in snippet view article find links to article

Delta Trianguli, Latinized from Delta Tri, is a spectroscopic binary star system approximately 35 light-years (11 pc) away in the constellation of Triangulum